The initial conditions of the universe: how much isocurvature is allowed?
classification
🌌 astro-ph
gr-qchep-th
keywords
alloweddirectionsnon-adiabaticadiabaticbaryoncancellationsconditionsconstraints
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We investigate the constraints imposed by the current data on correlated mixtures of adiabatic and non-adiabatic primordial perturbations. We discover subtle flat directions in parameter space that tolerate large (~60%) contributions of non-adiabatic fluctuations. In particular, larger values of the baryon density and a spectral tilt are allowed. The cancellations in the degenerate directions are explored and the role of priors elucidated.
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